(a) Find the total power radiated into space by the Sun
vher2gz0 p-m 6, assuming it to be a perfect emit
e-mp gvhr z620ter at $T\,=\,5500K$ The Sun’s radius is $7.0 \times10^{ 8}\,m$
$ \times10^{ 26}\,W$
(b) From this, determine the power per unit area arriving at the Earth, $1.5 \times10^{ 11}\,m$ away (Fig. 14–21).
$ \times10^{ 3}\,W/m^2$